| dc.contributor.advisor | Branch, David, | en_US |
| dc.contributor.author | Fisher, Adam Keith. | en_US |
| dc.date.accessioned | 2013-08-16T12:30:49Z | |
| dc.date.available | 2013-08-16T12:30:49Z | |
| dc.date.issued | 2000 | en_US |
| dc.identifier.uri | https://hdl.handle.net/11244/5920 | |
| dc.description.abstract | This work describes how to use and modify the highly parameterized spectrum synthesis code (SYNNEW). SYNNEW can be used to derive information directly from type Ia supernovae spectra. | en_US |
| dc.format.extent | v, 159 leaves : | en_US |
| dc.subject | Supernovae Spectra. | en_US |
| dc.subject | Supernovae. | en_US |
| dc.subject | Physics, Astronomy and Astrophysics. | en_US |
| dc.subject | Red shift. | en_US |
| dc.title | Direct analysis of type Ia supernovae spectra. | en_US |
| dc.type | Thesis | en_US |
| dc.thesis.degree | Ph.D. | en_US |
| dc.thesis.degreeDiscipline | Homer L. Dodge Department of Physics and Astronomy | en_US |
| dc.note | Adviser: David Branch. | en_US |
| dc.note | Source: Dissertation Abstracts International, Volume: 61-02, Section: B, page: 0891. | en_US |
| ou.identifier | (UMI)AAI9962949 | en_US |
| ou.group | College of Arts and Sciences::Homer L. Dodge Department of Physics and Astronomy | |
